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The Role of Three-Dimensional Geometry on Turbulence in Quasi-Helically Symmetric Stellarators

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서명/저자사항The Role of Three-Dimensional Geometry on Turbulence in Quasi-Helically Symmetric Stellarators.
개인저자Faber, Benjamin J.
단체저자명The University of Wisconsin - Madison. Physics.
발행사항[S.l.]: The University of Wisconsin - Madison., 2018.
발행사항Ann Arbor: ProQuest Dissertations & Theses, 2018.
형태사항207 p.
기본자료 저록Dissertation Abstracts International 79-12B(E).
Dissertation Abstract International
ISBN9780438269040
학위논문주기Thesis (Ph.D.)--The University of Wisconsin - Madison, 2018.
일반주기 Source: Dissertation Abstracts International, Volume: 79-12(E), Section: B.
Advisers: Chris C. Hegna
요약The ability to optimize stellarator geometry to reduce transport has led to renewed interest in stellarators for magnetic confinement fusion. In this thesis, turbulence in the Helically Symmetric eXperiment (HSX), a quasi-helically symmetric ste
요약The first comprehensive simulations of Trapped Electron Mode turbulence in HSX are presented. HSX geometry introduces a complex landscape of unstable eigenmodes, with strongly ballooning modes, non-symmetric modes, and extended modes all coexist
요약These linear and nonlinear features are the consequence of the low global magnetic shear of HSX, which allows modes to extend far along field lines and requires simulation domains spanning multiple poloidal turns to properly resolve. Subdominant
일반주제명Plasma physics.
Physics.
언어영어
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